SHINE: Digitization of 27 Years of Big Bear Solar Observatory (BBSO) Films and Application in Statistical Study of Filaments and Flares

SHINE:大熊太阳天文台 (BBSO) 27 年胶片的数字化及其在灯丝和耀斑统计研究中的应用

基本信息

  • 批准号:
    0849453
  • 负责人:
  • 金额:
    $ 39.13万
  • 依托单位:
  • 依托单位国家:
    美国
  • 项目类别:
    Continuing Grant
  • 财政年份:
    2009
  • 资助国家:
    美国
  • 起止时间:
    2009-03-01 至 2014-02-28
  • 项目状态:
    已结题

项目摘要

From 1969 to 1995, Big Bear Solar Observatory (BBSO) staff recorded all of their observations on 35 mm film before switching to digital imaging after 1995. These film data include full-disk observations from BBSO's 8 inch telescope and high resolution observations from the 10 and 26 inch telescopes, with the cadence of observations ranging from 10 seconds to 1 minute. These film data cover two and one-half solar cycles, include thousands of flares, and span the entire operational service of several space missions, including SMM, CGRO, and Yohkoh. Wide public access to these BBSO data films is impractical and their scientific capability has never been fully explored. The requested funding will support the purchase of specialized commercial digitizing equipment, as well as the employment of a postdoctoral researcher and undergraduate students to digitize these films and archive them in the public domain. The BBSO data to be digitized includes full-disk and high resolution H-alpha images, as well as He I images. The entire set of full-disk data will be converted to create a synoptic data base. High resolution film data will be digitized according to events selected by the full-disk data. All observed solar flares and filament eruptions will be automatically detected and cataloged using artificial intelligence methods that have been developed and implemented at BBSO. Despite some limitations of the film data format, the PI notes that the long-term coverage and high quality of the BBSO data will have very broad applications for many statistical studies. The PI's team will carry out targeted research on the filaments and flares with the digitized data. They plan to perform statistical analysis of solar filaments, including their motions and eruptions. They will study filament oscillations to verify whether they are precursors to, or the result of, solar flares. The PI and postdoc will investigate the rate of magnetic reconnection at the Sun and the relationship of filament acceleration to hard X-ray (HXR) emission. This new study will complement the ongoing comparison of existing BBSO digital data and HXR data from the RHESSI spacecraft.This research addresses the SHINE goal of understanding the initiation of CMEs and electron acceleration in flares. The study of a large number of archived events will improve the forecasting of future solar eruptive events, and thus assist operational space weather prediction. Funding is not requested for the PI, but it will instead support the postdoc and undergraduate students. At least three undergraduate students will participate in the film digitization and research, and the postdoc will gain management training by assisting the PI in supervising these students.
从1969年到1995年,大熊太阳天文台(BBSO)的工作人员在35毫米胶片上记录了他们所有的观测结果,1995年后改用数字成像。这些胶片数据包括BBSO 8英寸望远镜的全磁盘观测和10英寸和26英寸望远镜的高分辨率观测,观测的节奏从10秒到1分钟不等。这些电影数据涵盖了两个半太阳周期,包括数千次耀斑,并涵盖了几个太空任务的整个操作服务,包括SMM,CGRO和Yohkoh。广泛的公众访问这些BBSO数据电影是不切实际的,他们的科学能力从来没有得到充分的探索。申请的资金将用于购买专门的商业数字化设备,以及雇用一名博士后研究人员和本科生对这些电影进行数字化处理并将其存档在公共领域。数字化的BBSO数据包括全磁盘和高分辨率H-α图像,以及He I图像。整套完整的磁盘数据将被转换成一个天气数据库。高分辨率胶片数据将根据全磁盘数据选择的事件进行数字化。所有观测到的太阳耀斑和暗条喷发都将使用BBSO开发和实施的人工智能方法自动检测和编目。尽管电影数据格式存在一些局限性,但PI指出,BBSO数据的长期覆盖范围和高质量将在许多统计研究中得到非常广泛的应用。PI的团队将利用数字化数据对细丝和耀斑进行有针对性的研究。他们计划对太阳细丝进行统计分析,包括它们的运动和爆发。他们将研究暗条振荡,以验证它们是否是太阳耀斑的前兆或结果。PI和博士后将研究太阳磁场重联的速率以及暗条加速与硬X射线(HXR)发射的关系。这项新的研究将补充现有BBSO数字数据和RHESSI航天器HXR数据的持续比较。这项研究解决了SHINE的目标,即理解CME的启动和耀斑中的电子加速。对大量存档事件的研究将改进对未来太阳爆发事件的预测,从而有助于空间气象的实用预测。PI不需要资金,但它将支持博士后和本科生。至少有三名本科生将参与电影数字化和研究,博士后将通过协助PI监督这些学生来获得管理培训。

项目成果

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Haimin Wang其他文献

Effects of the phase content on dynamic damage evolution in Fe50Mn30Co10Cr10 high entropy alloy
相含量对Fe50Mn30Co10Cr10高熵合金动态损伤演化的影响
  • DOI:
    10.1016/j.jallcom.2020.156883
  • 发表时间:
    2021-01
  • 期刊:
  • 影响因子:
    6.2
  • 作者:
    Yang Yang;Shuangjun Yang;Haimin Wang
  • 通讯作者:
    Haimin Wang
Efficient reprogramming of the heavy-chain CDR3 regions of a human antibody repertoire
人抗体库重链 CDR3 区的有效重编程
  • DOI:
    10.1101/2021.04.01.437943
  • 发表时间:
    2021
  • 期刊:
  • 影响因子:
    0
  • 作者:
    T. Ou;Wenhui He;Brian D. Quinlan;Yan Guo;P. Karunadharma;Hajeung Park;Meredith E. Davis;Mai H. Tran;Yiming Yin;Xia Zhang;Haimin Wang;Guocai Zhong;M. Farzan
  • 通讯作者:
    M. Farzan
RELATIONSHIP BETWEEN CME KINEMATICS AND FLARE STRENGTH
CME 运动学与耀斑强度之间的关系
  • DOI:
  • 发表时间:
    2003
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Y. Moon;G. Choe;Haimin Wang;Y. Park;C. Cheng
  • 通讯作者:
    C. Cheng
Solar activity monitoring and forecasting capabilities at Big Bear Solar Observatory
大熊太阳观测站的太阳活动监测和预报能力
  • DOI:
    10.5194/angeo-20-1105-2002
  • 发表时间:
    2002
  • 期刊:
  • 影响因子:
    1.9
  • 作者:
    P. Gallagher;C. Denker;V. Yurchyshyn;T. Spirock;J. Qiu;Haimin Wang;P. Goode
  • 通讯作者:
    P. Goode
Statistical Correlations between Parameters of Photospheric Magnetic Fields and Coronal Soft X-Ray Brightness
光球磁场参数与日冕软X射线亮度的统计相关性
  • DOI:
    10.1086/519304
  • 发表时间:
    2007
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Changyi Tan;J. Jing;V. Abramenko;A. Pevtsov;Hui Song;Sung;Haimin Wang
  • 通讯作者:
    Haimin Wang

Haimin Wang的其他文献

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{{ truncateString('Haimin Wang', 18)}}的其他基金

Collaborative Research: DKIST Critical Science: Study of Flare Producing Active Regions with Highest Resolution Observations and Data-based Magnetohydrodynamics (MHD) Modeling
合作研究:DKIST 关键科学:利用最高分辨率观测和基于数据的磁流体动力学 (MHD) 建模研究耀斑产生的活动区域
  • 批准号:
    2204384
  • 财政年份:
    2022
  • 资助金额:
    $ 39.13万
  • 项目类别:
    Standard Grant
Collaborative Research: SHINE: Investigation of Mini-filament Eruptions and Their Relationship with Small Scale Magnetic Flux Ropes in Solar Wind
合作研究:SHINE:研究太阳风中的微型细丝喷发及其与小规模磁通量绳的关系
  • 批准号:
    2229064
  • 财政年份:
    2022
  • 资助金额:
    $ 39.13万
  • 项目类别:
    Standard Grant
Collaborative Research: Dynamic and Non-Force-Free Properties of Solar Active Regions and Subsequent Initiation of Flares
合作研究:太阳活动区域的动态和非无力特性以及随后耀斑的引发
  • 批准号:
    1954737
  • 财政年份:
    2020
  • 资助金额:
    $ 39.13万
  • 项目类别:
    Standard Grant
EarthCube Data Capabilities: Machine Learning Enhanced Cyberinfrastructure for Understanding and Predicting the Onset of Solar Eruptions
EarthCube 数据功能:机器学习增强的网络基础设施,用于理解和预测太阳喷发的发生
  • 批准号:
    1927578
  • 财政年份:
    2019
  • 资助金额:
    $ 39.13万
  • 项目类别:
    Standard Grant
Collaborative Research: SHINE: Study of Long-Term Variability of Solar Chromospheric Activity in Multiple Solar Cycles
合作研究:SHINE:多个太阳周期中太阳色层活动的长期变化研究
  • 批准号:
    1620875
  • 财政年份:
    2016
  • 资助金额:
    $ 39.13万
  • 项目类别:
    Continuing Grant
High Resolution Observations of Evolution of Magnetic Fields and Flows Associated with Solar Eruptions
与太阳喷发相关的磁场和气流演化的高分辨率观测
  • 批准号:
    1408703
  • 财政年份:
    2014
  • 资助金额:
    $ 39.13万
  • 项目类别:
    Continuing Grant
Collaborative Research: SHINE: Laboratory, Observational, and Modeling Investigations of the Torus Instability and Associated Solar Corona Eruptive Phenomena
合作研究:SHINE:环面不稳定性和相关日冕喷发现象的实验室、观测和建模研究
  • 批准号:
    1348513
  • 财政年份:
    2014
  • 资助金额:
    $ 39.13万
  • 项目类别:
    Continuing Grant
Exploring Large-Scale Current Sheets Associated with Coronal Mass Ejections
探索与日冕物质抛射相关的大规模电流片
  • 批准号:
    1153226
  • 财政年份:
    2012
  • 资助金额:
    $ 39.13万
  • 项目类别:
    Standard Grant
Operation and Application of High-Resolution Full-Disk Global Halpha Network
高分辨率全盘全球Halpha网络的运行与应用
  • 批准号:
    0839216
  • 财政年份:
    2009
  • 资助金额:
    $ 39.13万
  • 项目类别:
    Continuing Grant
ATI: Adaptive Optics System for 1.6-m Solar Telescope in Big Bear
ATI:Big Bear 1.6 米太阳望远镜的自适应光学系统
  • 批准号:
    0604021
  • 财政年份:
    2006
  • 资助金额:
    $ 39.13万
  • 项目类别:
    Continuing Grant

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